核子结构函数探讨

本文利用文献[1]的方法讨论了核子结构函数, 并与不同Q²下的实验数据相比较, 其结果表明从强子波函数获得核子结构函数的理论方法是探讨强子结构函数初始条件的可能途径.     

极化光子的结构函数

在满足有非齐次项的演化方程的假定下, 求出了极化光子的分布函数和碎裂函数的矩. 然后利用雅可比多项式作级数展开, 求出了它们的用多项式表示的明显形式, 并具体给出了三项式, 五项式及七项式表示.     

Mechanism of Proton-Induced Reactions on Targets ^16O, ^27Al, ^56Fe, ^112Cd, ^184W and ^208Pb At Ep = 800 MeV

We investigate the 800 MeV proton-induced spallation reactions on various targets by the improved quantum molecular dynamics （ImQMD05） model incorporated with a statistical decay model （SDM）. The influence of the nucleon-nucleon effective interaction on proton induced spallation reactions is studied by using different Skyrme interactions. It is found that the low energy part of the neutron double differential cross sections （DDCS）, which is mainly contributed from the decay of the excited residue, is influenced by the effective nucleon-nucleon interaction strongly., while the high energy part of neutron DDCS is influenced weakly. Among the Skyrme interactions used in the calculations, the calculation results with SkP give the best agreement with the experimental data.     

光子结构函数的直接检验

本文基于喷注电荷截面方法,提出了一种直接测量光子结构函数的可行方案。 关键词：     

强子结构函数的数值解法

为了避免矩方法求解强子结构函数时对函数待定形式的依赖并提高解的精确度,本文采用把A-P方程离散为常微分方程组,用龙格-库塔方法求解的方法,得出随Q²变化的价夸克、海夸克和胶子的结构函数。     

氘核极化结构函数的核效应

极化深度非弹性散射是研究质子、氘核内部部分子精细结构的有利工具.利用基于微扰QCD模型得到的6夸克集团内部自旋夸克的分布函数,研究了氘核极化结构函数的核效应.发现考虑了核效应后的氘核极化结构函数比没有考虑核效应的结果能更好地符合SLAC E155的实验数据.     

基于结构函数方法的类星体证认

光变巡天是搜寻类星体的一个很有效的方法.应用归一化结构函数对SDSS stripe 82中存在光变的1411个类星体和174个恒星进行分类,选取幂函数模型拟合这些样本5个波段的结构函数.综合幅值和幂指数两个物理量设置了合适的分类判据,获得了比较理想的分类结果,类星体和恒星最高分类正确率分别达到了92.2%和83.6%.结果表明,改正后的结构函数对类星体的证认有很好的效果,能节约大型望远镜宝贵的观测时间,让类星体巡天获得比较高的观测效率.分析结论支持大部分类星体的光变缘于盘的不稳定性.     

Neutrino Energy Loss by Electron Capture on Nucleus ^56Mn, ^56Fe, ^56Co and ^56Ni in Strong Electron Screening

Based on the p-f shell model, the neutrino energy loss rates for nucleus ^56Mn, ^56Fe, ^56Co and ^56Ni in the electron capture process are canvassed in and not in a strong electron screening. The results show that the neutrino energy loss rates for ^56Mn, ^56Fe, ^56Co and ^56Ni decrease about 15%, 10%, 60% and i order of magnitude correspondingly at the temperature T9 = 15 and even debase 2 orders of magnitude at the temperature T9 = 1.     

袋的整体运动与核子结构函数

利用具有平移不变性的口袋-夸克波函数以及引入一个洛仑兹不变的有效拉氏函数,我们计算了核子深度非弹结构函数。在我们的计算中,4-动刃守恒自动满足,得到的结构函数正定且在ξ>1时为零。进一步利用渐近自由假设,我们获得了显示的Bjorken标度性及近似表达式F₁（ξ≈1）∝（1一ξ）⁴,顺便还得到一个新的计数法则。上机运算给出的F₂（ξ）曲线看来在区间0.4?ξ≤1内与实验数据相符。     

New Astrophysical Reaction Rates for ^18F（P,α）^15O and ^18F（P,γ）^19Ne

The rates of the thermonuclear ^18F(P,α)^15O and ^18F(P,γ)^19Ne reactions in hot astrophysical environments are needed to understand gamma-ray emission from nova explosions. The rates for these reactions have been uncertain due to discrepancies in recent measurements, as well as to a lack of a comprehensive examination of the available structure information in the compound nucleus ^19Ne. We have examined the latest experimental measurements with radioactive and stable beams, and made estimates of the unmeasured ^19Ne nuclear level parameters, to generate new rates with uncertainties for these reactions. The rates are expressed as numerical values over the temperature range relevant for stellar explosions, as well as analytical expressions as functions of temperature in a format suitable for use in astrophysical simulations. Comparisons with the previous rate calculations are carried out, and the astrophysical implications are briefly discussed.     

Optical Potential Parameters for Halo Nucleus System ^6He＋^12C from Transfer Reaction ^11B（^7Li, ^6He）^12C

The optical potential parameters for the halo nucleus system ^6He＋^12C are extracted from fits to the measured angular distributions of ^11B（^7Li, ^6He）12C reaction at energies of 18.3 and 28.3MeV with distorted-wave Born approximation analysis. The characters of the obtained optical potentiM parameters are basically consistent with the results extracted from the fits to the elastic-scattering angular distributions in the literature.     

干涉截面对核子自旋结构函数的影响

利用非相对论和相对论夸克模型分别计算了干涉截面对极化核子自旋结构函数的影响.计算所得到的明显的作用为今后实验上抽取核子自旋结构函数提供了依据.     

Randon变换在区域结构函数坍陷中的应用

为了更好地利用区域结构函数评价大口径反射镜表面面形,引入了Randon变换作为区域结构函数坍陷的工具。对于使用Randon变换进行区域结构函数坍陷的具体实现方法进行了讨论;之后考虑到Zernike多项式可以很好地模拟系统的低阶波像差,故利用此方法对于Zernike多项式的区域结构函数进行坍陷;然后将此方法应用于米级口径的反射镜表面面形检测数据以及30m望远镜(TMT)三镜面形仿真数据,验证了理论的正确性与方法的可行性。对于大口径反射系统的设计、检测与加工都有较好的指导意义,同时为30m望远镜三镜项目的最终完成提供助力。     

利用手征SU(3)夸克模型研究轻双Λ超核^6_ΛΛHe,^5_ΛΛHe,^5_ΛΛH,^4_ΛΛHe,和^4_ΛΛH的结合能

在手征SU(3)夸克集团模型下, 通过共振群方法(RGM)计算了双Λ超核^6_ΛΛHe,^5_ΛΛHe,^5_ΛΛH,^4_ΛΛHe,和^4_ΛΛH的结合能. 结果表明, 假定双Λ超核具有双Λ集团和壳心核集团构成的两集团结构, 得到的^6_ΛΛHe超核的结合能与实验值基本吻合, 表明手征SU(3)夸克集团模型不仅能较好地描述重子谱、N-N和Y-N相互作用及轻Λ超核的结合能, 也能较好地描述Y-Y相互作用及双Λ超核^6_ΛΛHe,^5_ΛΛHe,^5_ΛΛH,^4_ΛΛHe,和^4_ΛΛH的结合能, 指出了它们存在的可能性.     

Properties of the Alpha Decay Chain Nuclei of ^310 126, ^292 120 and ^298 114

The properties of the a decay nuclei of^310 126, ^292 120 and ^298 114 are investigated in the deformed relativistic meanfield model. The nuclear properties are investigated with the TMA and NL-Z2 parameter sets, and compared with Moller‘s result [At. Data Nucl. Data Tables 59 (1995) 185]. The results show that the a decay energy increases systematically with the increasing proton number. Meanwhile, the a decay energy has a minimum value at the point of shell closure. It is also found that among the three nuclei, ^292 120 is more possible to be the next doubly magic nucleus.